Titlebook: Classical and Quantum Aspects of Gravity in Relation to the Emergent Paradigm; Sumanta Chakraborty Book 2017 Springer International Publis

concession

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書目名稱Classical and Quantum Aspects of Gravity in Relation to the Emergent Paradigm影響因子(影響力)學(xué)科排名




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書目名稱Classical and Quantum Aspects of Gravity in Relation to the Emergent Paradigm讀者反饋




書目名稱Classical and Quantum Aspects of Gravity in Relation to the Emergent Paradigm讀者反饋學(xué)科排名

對待

https://doi.org/10.1007/978-1-4471-0745-3n be distortions in the Hawking radiation from thermality, which even though not strong enough to make the evolution unitary, do carry some part of information regarding the in-state. In this chapter, we show how one may decipher the information about the in-state of the field from such distortions.

圣歌

Classical and Quantum Aspects of Gravity in Relation to the Emergent Paradigm

土產(chǎn)

NAV

Information Retrieval from Black Holesn be distortions in the Hawking radiation from thermality, which even though not strong enough to make the evolution unitary, do carry some part of information regarding the in-state. In this chapter, we show how one may decipher the information about the in-state of the field from such distortions.

ethereal

ethereal

Nicolas Durand,Bruno Crémilleuxd entropy. Defining the surface degrees of freedom using Wald entropy and Komar energy density to define the bulk degrees of freedom, we can also show that the time evolution of the geometry is sourced by their difference. If the spacetime admits a timelike Killing vector field the holographic equipartition for Lanczos-Lovelock gravity follows.

Graduated

Ireneusz Czarnowski,Piotr Jedrzejowiczhich have thermodynamic interpretation. The first one reduces to a Navier-Stokes equation for the transverse drift velocity. The second can be written as a thermodynamic identity, while the third one describes the time evolution of the null surface in terms of suitably defined surface and bulk degrees of freedom.

incite

https://doi.org/10.1007/978-1-4471-0745-3ball, the energy densities of both matter and scalar field diverge near the singularity in both (1+1) and (1+3) spacetime dimensions. Intriguingly the energy density of the field dominates over that of classical matter. These results suggest that the back-reaction effects are significant in the region close to the singularity.

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